Statistics – Computation
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh41c..05z&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SH41C-05
Statistics
Computation
[7959] Space Weather / Models
Scientific paper
Understanding the acceleration of particles at interplanetary shocks is a cornerstone of anticipated space weather models. We will present a critical overview of the current status of the underlying physical processes, describe the translation of these processes into viable computational models, and then critically evaluate the application of these models to a series of carefully chosen observations. Of critical importance is the recognition that the acceleration process is highly dynamical and that our simple ideas based on steady-state models do not serve as a good guide to observations. The importance of shock geometry will be stressed, and our current ideas about the “injection” of particles into the acceleration process will be survey briefly. Finally, in view of the critical role that turbulence plays in the transport of particles once accelerated, we will discuss turbulence transport models within about 5 AU.
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